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• Main Page
  {{DISPLAYTITLE:Planck 2015 Release Explanatory Supplement}} ...="color:Blue"> This is the Explanatory Supplement development page for the Planck 2015 data release </span>
  6 KB (669 words) - 21:21, 6 August 2018
• LFI design, qualification, and performance
  ...ng a further radio frequency amplification stage, detector diodes, and all the electronics for data acquisition and bias supply. ...ng to the HFI helium J-T cooler. Two sorption cooler units are included in the flight hardware.
  50 KB (7,826 words) - 22:29, 4 February 2015
• The HFI DPC
  ...3 can rely on simulation provided by the LS, while L4 refers to delivering the DPC products to ESA. This processing relies on dedicated software and hard ...and its companion papers provide the reference for the processing done for the 2013 data release.
  4 KB (627 words) - 13:09, 7 July 2015
• The LFI DPC
  ...lly Level 4 merely acts to reformat, document and deliver the products to the final archive (PLA). ...eration Centre). Level 1 uses TM data for performing a routine analysis of the S/C and P/L
  8 KB (1,072 words) - 20:27, 4 February 2015
• Simulation data
  ...ogether with separate sets of Monte Carlo realizations of the CMB and the instrument noise. Currently, only a subset of these simulations is available from the Planck Legacy Archive. In particular:
  46 KB (7,032 words) - 12:02, 29 March 2016
• Catalogues
  ...S]] and in section 2 of {{PlanckPapers|planck2014-a35}}. The validation of the catalogues is described in section 3 of {{PlanckPapers|planck2014-a35}}. ...catalogues; PCCS2, here the detected sources are located in regions of the sky where it is not possible to make an estimate of their reliability.
  72 KB (10,038 words) - 08:40, 24 October 2016
• CMB spectrum & Likelihood Code
  ...rs associated with this spectrum are the 68% confidence limits and include the uncertainties due to foreground subtraction. ...eam uncertainties. Both Commander and Plik are described in more detail in the sections below.
  61 KB (9,011 words) - 08:06, 15 May 2017
• Glossary
  * '''4-K lines''': EMI/EMC influence of the 4-K cooler mechanical motion on the bolometer readout electronics. *'''bandpass''': same as the spectral response.
  7 KB (1,093 words) - 13:07, 7 July 2015
• Timelines
  ...er quantity giving the value of that quantity as a function of time during the mission. For LFI, refer to {{PlanckPapers|planck2014-a03}}, and for HFI, t ...ned and calibrated signal and 3 timelines of coordinates, corresponding to the two angular coordinates and one position angle.
  28 KB (4,415 words) - 18:43, 21 August 2015
• Sky temperature maps
  {{DISPLAYTITLE:2015 Sky temperature and polarization maps}} ...ection). The details of the start and end of the time ranges are given in the table below.
  45 KB (6,681 words) - 11:55, 16 May 2017
• Map-making
  ...on procedures used by the HFI DPC to build detector and frequency maps for the 2015 data release. They are described in {{PlanckPapers|planck2014-a09}}. These have common elements with the tools used for the 2013 release that are described in {{PlanckPapers|planck2013-p03}} and {{P
  12 KB (1,956 words) - 12:56, 7 July 2015
• The RIMO
  {{DISPLAYTITLE:The 2015 instrument model}} ...me overall structure, but will differ in the details. The type of data in the RIMO can be:
  14 KB (2,168 words) - 09:15, 8 March 2017
• TOI processing LFI
  ...s from one diode are combined with signals from the complementary diode in the same radiometer. Finally, photometric calibration is applied for each horn. ...nd data sampling divisions are stored in the database, in order to improve the analysis.
  34 KB (5,468 words) - 15:34, 4 February 2015
• Map-making LFI
  ...to the mapmaking procedure consist of the calibrated timelines, along with the corresponding pointing information. The main output consists of temperature and polarization maps.
  26 KB (3,949 words) - 15:33, 1 March 2017
• Beams LFI
  LFI observed the sky with 11 pairs of beams associated with the 22 pseudo-correlation radiometers. ...28; M and S are the two polarizations, namely the main-arm and side-arm of the Orthomode transducers {{BibCite|darcangelo2009b}} (see also [[LFI design, q
  24 KB (3,748 words) - 10:02, 26 September 2016
• References
  author = {Planck Collaboration I,}, title = {Planck 2013 results: Overview of Planck Products and Scientific Results (p01)},
  173 KB (25,381 words) - 15:29, 4 June 2014
• LFI-Validation
  ...data validation is based on null tests. Here we present some examples from the current release, with comments on relevant time scales and sensitivity to v Null tests at map level are performed routinely, whenever changes are made to the mapmaking pipeline. These include differences at survey, year, 2-year, hal
  10 KB (1,699 words) - 13:37, 19 September 2016
• HL-sims
  ...ke in actual band-passes (in a RIMO) and create sky maps and catalogues at the specified frequencies. It can be supplemented by ad-hoc simulation software ...Alternatively, the output can be used as input to a detailed simulation of the instrumental behaviour.
  5 KB (779 words) - 16:03, 21 May 2014
• Mission products
  {{DISPLAYTITLE:Planck 2015 Mission products}} The products of the Planck mission that are made public at this time and described in this document co
  3 KB (438 words) - 10:45, 5 February 2015
• Spectral response
  ...3d}} and [[HFI_cold_optics#Spectral_response|here]] for the description of the spectral response pre-launch measurements). ...erties of the individual detectors, and band-averaged spectra, is shown at the bottom of this page.
  21 KB (1,186 words) - 12:57, 7 July 2015
• Compact Source catalogues
  ==Planck Catalogue of Compact Sources== ...ency lists of sources, both Galactic and extragalactic, extracted from the Planck maps.
  25 KB (3,934 words) - 15:07, 26 September 2016
• HFI detection chain
  ...of the HFI - the detectors - are bolometers, solid-state devices in which the incoming radiation dissipates its energy as heat that increases the temperature of a
  14 KB (2,155 words) - 23:49, 12 November 2014
• Effective Beams
  ...etry of the beam and the uneven distribution of scanning angles across the sky. ..., the objects whose convolution with the true CMB sky produce the observed sky map.
  22 KB (3,180 words) - 10:37, 5 February 2015
• Main Page3
  #[[The Planck mission|The Planck mission]] <span style="color:red">(Dupac)</span> #[[The satellite|The satellite]]
  6 KB (770 words) - 17:33, 29 January 2013
• List of acronyms
  * '''DMC''' : Data Management Component, the databases used at the HFI and LFI DPCs * '''FLS ''' : (Planck) First Light Survey
  6 KB (650 words) - 23:43, 1 February 2015
• LFI systematic effect uncertainties
  ...are dependent on the sky and that cannot be considered independently from the observation strategy. ...und in {{PlanckPapers|planck2013-p02a}} and {{PlanckPapers|planck2014-a04||Planck-2015-A04}}.
  20 KB (2,907 words) - 13:28, 19 September 2016
• References2
  author = {Planck Collaboration XXXI,}, title = {Planck 2013 results: All-sky model of thermal dust emission},
  39 KB (5,438 words) - 09:40, 20 May 2014
• LFIAppendix
  ...h component of the LFI instrument, which were already briefly described in the main [[LFI design, qualification, and performance|LFI instrument]] page. ...mposed of a sine-squared profiled section, and an exponential profile near the aperture plane.
  60 KB (9,314 words) - 08:48, 2 January 2015
• Frequency maps angular power spectra
  {{DISPLAYTITLE:Sky temperature power spectra}} Angular power spectra of cut sky CMB dominated maps are provided to allow independent cosmological analysis
  25 KB (3,718 words) - 15:37, 18 July 2014
• Astrophysical component separation
  See the Component Separation paper {{PlanckPapers|planck2013-p06}} {{PlanckPapers|p ...' which are spherical wavelets. A special procedure is used for processing the coarsest needlet scale
  14 KB (2,212 words) - 15:15, 26 September 2016
• Astrophysical component maps test
  We describe diffuse foreground products for the Planck 2013 release. See Planck paper P06-Component Separation <cite>#planck2013-p06</cite> for a detailed ...e result of the fitting for one foreground component at low frequencies in Planck bands,
  22 KB (2,713 words) - 18:48, 1 March 2013
• Beams
  = The 2015 Data Release = ...tions of Uranus and Neptune are used to obtain an absolute calibration for the 545 and 857 GHz channels.
  52 KB (8,515 words) - 12:52, 7 July 2015
• CMB and astrophysical component maps
  ...how it is obtained, followed by a description of the FITS file containing the data and associated information. All the details can be found in {{PlanckPapers|planck2014-a11}} and {{PlanckPapers|
  90 KB (13,248 words) - 13:06, 21 April 2020
• Changelog
  * 2013-04-03, Mendes. [[Sky temperature maps]]: fixed incorrect links (Ticket ID DTX-918825). <span sty ...Mendes, [[CMB and astrophysical component maps]]: Fixed incorrect links to the new nilc and smica CMB maps. <span style="color:Green">Moved to public ES.<
  12 KB (1,788 words) - 08:42, 25 September 2014
• TOC WorkInProgress
  ##[[The Planck mission_WiP|The Planck mission]] ##[[The satellite_WiP|The satellite]]
  5 KB (581 words) - 09:33, 31 March 2014
• TOCV1 BackUp
  #[[The Planck mission|The Planck mission]] (<span style="color:red">Dupac</span>,<span style="color:blue">Le #[[The satellite|The satellite]](<span style="color:red">Dupac</span>,<span style="color:blue">M
  6 KB (744 words) - 09:45, 31 March 2014
• TestMassEditing
  ...ngstatics | this table]]. As a secondary product, maps with estimates of the Zodiacal light and Far-Side-Lobes contribution removed are also provided. ...s the maps themselves and of other products described elsewhere (see e.g., the [[HFI-Validation | data validation]] section).
  35 KB (5,146 words) - 17:59, 3 July 2014
• TestReplace2
  ...of the HFI - the detectors - are bolometers, solid-state devices in which the incoming radiation dissipates its energy as heat that increases the temperature of a
  13 KB (2,128 words) - 15:29, 4 June 2014
• Terminology
  ;4K lines: EMI/EMC influence of the 4K cooler mechanical motion on the bolometer readout electronics. ...led spectral energy distributions or well known spectra, and requires that the detector's spectral bandpass also be well known.
  10 KB (1,539 words) - 15:11, 21 July 2014
• NoiseCovarMatrices
  ...matrix is required for maximum likelihood analysis of CMB anisotropies in the maps but also for low resolution component separation. ...detector noise. We do this for each detector at roughly one day intervals. The process is
  6 KB (1,020 words) - 18:38, 19 December 2014
• Planck Added Value Tools
  {{DISPLAYTITLE:Planck Added Value Tools Documentation}} ==General information about the functionality offered==
  30 KB (5,022 words) - 16:55, 16 March 2018